Overview of KAGRA: Detector design and construction history
Author:
Akutsu T12, Ando M343, Arai K1, Arai Y4, Araki S3, Araya A1, Aritomi N3, Aso Y15, Bae S4, Bae Y3, Baiotti L1, Bajpai R3, Barton M A1, Cannon K4, Capocasa E3, Chan M1, Chen C36, Chen K1, Chen Y4, Chu H3, Chu Y -K1, Eguchi S3, Enomoto Y1, Flaminio R43, Fujii Y3, Fukunaga M1, Fukushima M3, Ge G1, Hagiwara A47, Haino S3, Hasegawa K1, Hayakawa H3, Hayama K1, Himemoto Y4, Hiranuma Y3, Hirata N1, Hirose E3, Hong Z1, Hsieh B H4, Huang C -Z3, Huang P1, Huang Y3, Ikenoue B1, Imam S4, Inayoshi K3, Inoue Y1, Ioka K3, Itoh Y18, Izumi K4, Jung K3, Jung P1, Kajita T3, Kamiizumi M1, Kanda N48, Kang G3, Kawaguchi K1, Kawai N3, Kawasaki T1, Kim C4, Kim J C3, Kim W S1, Kim Y -M3, Kimura N1, Kita N4, Kitazawa H3, Kojima Y1, Kokeyama K3, Komori K1, Kong A K H4, Kotake K3, Kozakai C1, Kozu R3, Kumar R1, Kume J4, Kuo C3, Kuo H -S1, Kuroyanagi S3, Kusayanagi K1, Kwak K4, Lee H K3, Lee H W1, Lee R3, Leonardi M1, Lin L C -C4, Lin C -Y3, Lin F -L1, Liu G C3, Luo L -W1, Marchio M4, Michimura Y3, Mio N1, Miyakawa O3, Miyamoto A1, Miyazaki Y4, Miyo K3, Miyoki S1, Morisaki S3, Moriwaki Y1, Nagano K4, Nagano S3, Nakamura K1, Nakano H3, Nakano M19, Nakashima R4, Narikawa T3, Negishi R1, Ni W -T31011, Nishizawa A1, Obuchi Y4, Ogaki W3, Oh J J1, Oh S H3, Ohashi M1, Ohishi N4, Ohkawa M3, Okutomi K1, Oohara K3, Ooi C P1, Oshino S4, Pan K3, Pang H1, Park J3, Arellano F E Peña1, Pinto I4, Sago N3, Saito S1, Saito Y3, Sakai K1, Sakai Y4, Sakuno Y3, Sato S1, Sato T3, Sawada T1, Sekiguchi T4, Sekiguchi Y3, Shibagaki S1, Shimizu R3, Shimoda T1, Shimode K4, Shinkai H3, Shishido T1, Shoda A3, Somiya K1, Son E J4, Sotani H3, Sugimoto R112, Suzuki T3, Suzuki T1, Tagoshi H4, Takahashi H3, Takahashi R1, Takamori A3, Takano S1, Takeda H4, Takeda M3, Tanaka H1, Tanaka K3, Tanaka K1, Tanaka T4, Tanaka T3, Tanioka S15, Tapia San Martin E N3, Telada S1, Tomaru T4, Tomigami Y3, Tomura T1, Travasso F313, Trozzo L1, Tsang T4, Tsubono K3, Tsuchida S1, Tsuzuki T3, Tuyenbayev D1, Uchikata N4, Uchiyama T3, Ueda A1, Uehara T314, Ueno K1, Ueshima G4, Uraguchi F3, Ushiba T1, van Putten M H P M4, Vocca H3, Wang J1, Wu C4, Wu H3, Wu S1, Xu W- R4, Yamada T3, Yamamoto K1, Yamamoto K4, Yamamoto T3, Yokogawa K1, Yokoyama J41, Yokozawa T3, Yoshioka T1, Yuzurihara H4, Zeidler S3, Zhao Y1, Zhu Z -H4
Affiliation:
1. Department of Physics, The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan 2. Advanced Technology Center, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan 3. Gravitational Wave Science Project, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan 4. Research Center for the Early Universe (RESCEU), The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan 5. The Graduate University for Advanced Studies (SOKENDAI), Mitaka City, Tokyo 181-8588, Japan 6. Department of Physics and Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan 7. Applied Research Laboratory, High Energy Accelerator Research Organization (KEK), Tsukuba City, Ibaraki 305-0801, Japan 8. Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP), Osaka City University, Sumiyoshi-ku, Osaka City, Osaka 558-8585, Japan 9. Institute for Cosmic Ray Research (ICRR), KAGRA Observatory, The University of Tokyo, Kashiwa City, Chiba 277-8582, Japan 10. State Key Laboratory of Magnetic Resonance and Atomic and Molecular Physics, Innovation Academy for Precision Measurement Science and Technology (APM), Chinese Academy of Sciences, Xiao Hong Shan, Wuhan 430071, China 11. Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan 12. Graduate School of Science and Engineering, University of Toyama, Toyama City, Toyama 930-8555, Japan 13. Istituto Nazionale di Fisica Nucleare, University of Perugia, Perugia 06123, Italy 14. Department of Physics, University of Florida, Gainesville, FL 32611, USA
Abstract
Abstract
KAGRA is a newly built gravitational-wave telescope, a laser interferometer comprising arms with a length of 3 km, located in Kamioka, Gifu, Japan. KAGRA was constructed under the ground and it is operated using cryogenic mirrors that help in reducing the seismic and thermal noise. Both technologies are expected to provide directions for the future of gravitational-wave telescopes. In 2019, KAGRA finished all installations with the designed configuration, which we call the baseline KAGRA. For this occasion, we present an overview of the baseline KAGRA from various viewpoints in a series of articles. In this article, we introduce the design configurations of KAGRA with its historical background.
Publisher
Oxford University Press (OUP)
Subject
General Physics and Astronomy
Cited by
197 articles.
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